59 Cygni: A Tilted ϕ Persei like System
2000 ◽
Vol 175
◽
pp. 581-584
◽
Keyword(s):
AbstractThe binarity of 59 Cygni was confirmed and orbital parameters from the radial velocity curve of the primary derived. The observed emission variability resembles the one of ɸ Per in quite some detail, suggesting a similar nature of the companion: a hot, compact star.
2019 ◽
Vol 491
(4)
◽
pp. 5489-5497
◽
2012 ◽
Vol 45
(1)
◽
pp. 1-6
◽
Keyword(s):
1985 ◽
Vol 87
◽
pp. 109-115
Keyword(s):
1997 ◽
Vol 123
(2)
◽
pp. 209-218
◽
2004 ◽
Vol 194
◽
pp. 269-269
◽
1995 ◽
pp. 243-244
◽